Title of article :
A post-Galileo view of Ioʹs interior
Author/Authors :
Keszthelyi، نويسنده , , Laszlo and Jaeger، نويسنده , , Windy L. and Turtle، نويسنده , , Elizabeth P and Milazzo، نويسنده , , Moses and Radebaugh، نويسنده , , Jani، نويسنده ,
Issue Information :
روزنامه با شماره پیاپی سال 2004
Abstract :
We present a self-consistent model for the interior of Io, taking the recent Galileo data into account. In this model, Io has a completely molten core, substantially molten mantle, and a very cold lithosphere. Heat from magmatic activity can mobilize volatile compounds such as SO2 in the lithosphere, and the movement of such cryogenic fluids may be important in the formation of surface features including sapping scarps and paterae.
Keywords :
IO , volcanism , interiors
